Development of Monolithic CMOS Detectors as x-ray Imaging Spectrometers

被引:2
作者
Kenter, A. T. [1 ]
Kraft, R. [1 ]
Murray, S. S. [2 ]
机构
[1] Harvard Smithsonian Ctr Astrophys, 60 Garden St, Cambridge, MA 02138 USA
[2] Johns Hopkins Univ, Dept Phys & Astron, Baltimore, MD 21218 USA
来源
HIGH ENERGY, OPTICAL, AND INFRARED DETECTORS FOR ASTRONOMY V | 2012年 / 8453卷
关键词
D O I
10.1117/12.925145
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present preliminary results from our ongoing program to develop CMOS detectors as single photon counting, soft X-ray imaging spectrometers. The Smithsonian Astrophysical Observatory in collaboration with SRI International/Sarnoff has been developing monolithic CMOS detectors optimized for x-ray astronomy. Our latest detector consists of an array of 1k x 1k 16 mu m pixels manufactured on 15 mu m epitaxial Si. These detectors are designed to be packaged and thinned for back illumination. The devices have on-chip CDS and are optimized to have high (similar to 40 frame/sec) read-out rates. Such monolithic CMOS imaging sensors would be ideal candidate detectors for the focal planes of space-borne soft x-ray astronomy missions. The high through-put, low noise and excellent low energy response, provide high dynamic range and good time resolution; bright and time varying x-ray features could be temporally and spectrally resolved without saturation or photon pile-up.
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页数:14
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